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Article: Kinematics and dynamics of the galactic bulge through planetary nebulae

TitleKinematics and dynamics of the galactic bulge through planetary nebulae
Authors
KeywordsPlanetary nebulae
Dynamics
Kinematics
Issue Date2006
Citation
Proceedings of the International Astronomical Union, 2006, v. 2, n. 234, p. 485-486 How to Cite?
AbstractThe discovery of ∼500 planetary nebulae (PNe) in the bulge region allows us to probe the bulge out to ∼ 8 kpc. This opens up the possibility to track bulge-disc interactions to unprecedented details. We present an exploration of bulge dynamics with Nbody models of a triaxial bulge embedded in an exponential disc (Peyaud 2005). © 2006 International Astronomical Union.
Persistent Identifierhttp://hdl.handle.net/10722/208870
ISSN
2020 SCImago Journal Rankings: 0.124

 

DC FieldValueLanguage
dc.contributor.authorPeyaud, Alan E J-
dc.contributor.authorBoily, Christian M.-
dc.contributor.authorAcker, Agnes̀s-
dc.contributor.authorParker, Quentin A.-
dc.date.accessioned2015-03-23T02:02:00Z-
dc.date.available2015-03-23T02:02:00Z-
dc.date.issued2006-
dc.identifier.citationProceedings of the International Astronomical Union, 2006, v. 2, n. 234, p. 485-486-
dc.identifier.issn1743-9213-
dc.identifier.urihttp://hdl.handle.net/10722/208870-
dc.description.abstractThe discovery of ∼500 planetary nebulae (PNe) in the bulge region allows us to probe the bulge out to ∼ 8 kpc. This opens up the possibility to track bulge-disc interactions to unprecedented details. We present an exploration of bulge dynamics with Nbody models of a triaxial bulge embedded in an exponential disc (Peyaud 2005). © 2006 International Astronomical Union.-
dc.languageeng-
dc.relation.ispartofProceedings of the International Astronomical Union-
dc.subjectPlanetary nebulae-
dc.subjectDynamics-
dc.subjectKinematics-
dc.titleKinematics and dynamics of the galactic bulge through planetary nebulae-
dc.typeArticle-
dc.description.naturelink_to_subscribed_fulltext-
dc.identifier.doi10.1017/S1743921306003863-
dc.identifier.scopuseid_2-s2.0-33845533791-
dc.identifier.volume2-
dc.identifier.issue234-
dc.identifier.spage485-
dc.identifier.epage486-
dc.identifier.eissn1743-9221-
dc.identifier.issnl1743-9213-

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